Table A.1
Restframe UV-to-FIR photometry sets for our sample (AB magnitudes up to the IRAC bands included, then in mJy) with 1σ uncertainties.
| Observing band | C0 | h7 | HLS115 | nn4 | MACS0451a |
|
|
|||||
| B | 22.300 ± 0.104 | 23.298 ± 0.131 | 22.968 ± 0.048 | <26.60 | 20.838 ± 0.020 |
| g | − | − | − | 20.606 ± 0.045 | |
| V | − | − | − | 20.425 ± 0.020 | |
| F602W | − | − | − | 20.347 ± 0.020 | |
| R | − | 21.994 ± 0.050 | <26.28 | − | |
| r | − | − | − | 20.175 ± 0.050 | |
| F702W | 21.154 ± 0.083 | − | 21.896 ± 0.050 | − | − |
| i | − | − | − | 20.299 ± 0.076 | |
| Ic | − | − | − | 20.148 ± 0.020 | |
| F814W | 20.802 ± 0.078 | 21.602 ± 0.027 | 21.450 ± 0.060 | − | 20.062 ± 0.020 |
| z | − | 21.360 ± 0.053 | 21.144 ± 0.072 | 24.70 ± 0.21 | − |
| J/ISAAC | − | 20.104 ± 0.029 | 20.278 ± 0.049 | 22.98 ± 0.06 | − |
| F110W | 19.643 ± 0.031 | − | 19.675 ± 0.020 | ||
| F140W | − | − | − | 19.181 ± 0.020 | |
| F160W | 19.118 ± 0.030 | − | |||
| H/ISAAC | − | 19.775 ± 0.040 | 19.928 ± 0.052 | 22.33 ± 0.06 | − |
| Ks | 18.643 ± 0.091 | 19.470 ± 0.036 | 19.285 ± 0.030 | 21.45 ± 0.04 | − |
| IRAC 3.6 μm | 17.925 ± 0.061 | 18.635 ± 0.027 | 18.885 ± 0.029 | 20.53 ± 0.04 | 18.913 ± 0.020 |
| IRAC 4.5 μm | 17.693 ± 0.067 | 18.441 ± 0.038 | 18.677 ± 0.031 | 20.15 ± 0.04 | 18.898 ± 0.020 |
|
|
|||||
| MIPS 24 μm (mJy) | 0.945 ± 0.060 | 0.341 ± 0.060 | 0.69 ± 0.06 | <0.20 | − |
| PACS 100 μm (mJy) | 7.73 ± 0.38 | 8.37 ± 0.37 | 19.96 ± 0.37 | 8.58 ± 0.37 | 9.86 ± 0.60 |
| PACS 160 μm (mJy) | 31.26 ± 0.95 | 24.61 ± 0.95 | 41.48 ± 0.96 | 25.26 ± 0.95 | 17.67 ± 0.95 |
| SPIRE 250 μm (mJy) | 46.68 ± 1.68 | 40.16 ± 1.33 | 53.59 ± 1.75 | 45.30 ± 1.87 | 17.61 ± 3.18 |
| SPIRE 350 μm (mJy) | 39.88 ± 1.68 | 27.36 ± 1.48 | 37.84 ± 1.64 | 38.04 ± 2.19 | 11.27 ± 3.29 |
| SPIRE 500 μm (mJy) | 21.47 ± 1.13 | 12.01 ± 1.29 | 18.64 ± 1.22 | 17.74 ± 1.50 | 5.24 ± 2.69 |
| SCUBA2 850 μm (mJy) | 5.39 ± 0.23 | 3.26 ± 0.70 | − | 3.02 ± 0.65 | − |
Notes. B and R bands correspond to CFHT/12k for A68, whereas B, V, and Ic in the case of MACS0451 correspond to Subaru’s SuprimeCam. Ks photometry comes from UKIRT, z is from VLT/FORS2, and g, r, i from SDSS.
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